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MultiDark
Anti-Helium from Dark Matter Annihilations Arxiv:1401.4017V3 [Hep-Ph] 24 Aug 2016
The Boundary of Galaxy Clusters and Its Implications on SFR Quenching
Multi-Dark
Clustering and Halo Abundances in Early Dark Energy Cosmological Models
Arxiv:1208.6426V2 [Hep-Ph]
The Story of Dark Matter Halo Concentrations and Density Profiles
(CMB) Radiation Was First Detected
Pos(DSU 2012)044 Ce
A Robust and Efficient Deep Learning Method for Dynamical Mass Measurements of Galaxy Clusters
Arxiv:1305.3651V1 [Astro-Ph.CO] 15 May 2013 E Omn Ttendso Lmns Ist the to Fits Galaxy the to at and filaments
Giovanni Cantatore University and INFN Trieste - Italy
A Python Toolkit for Cosmology, Large-Scale Structure, and Dark Matter Halos
Weak Lensing Reveals a Tight Connection Between Dark Matter Halo Mass and the Distribution of Stellar Mass in Massive Galaxies
Predictions for JWST from the Universemachine DR1
[OII] Emitters in Multidark-Galaxies and DEEP2
Working Group Particles LHC + DM
Pos(DSU2015)030 ∗†
[email protected]
Speaker
Systematic Uncertainties from Halo Asphericity in Dark Matter Searches
Top View
Exploring the High-Mass End of the Stellar Mass Function of Star
Arxiv:1502.05703V2 [Hep-Ph] 31 Mar 2015 Discovered Soon
MULTIDARK-GALAXIES: Data Release and first Results
MPA Lecture on Numerical Methods for Cosmology
Aldo Morselli INFN Roma Tor Vergata
Darkmatter Groupe.Pdf
The Mare Nostrum Universe the Biggest SPH Simulation up To
Arxiv:2006.13231V2 [Astro-Ph.CO] 14 Mar 2021
Projected Sensitivity of the Supercdms SNOLAB Experiment
Early Growth in a Perturbed Universe: Exploring Dark Matter Halo Populations in 2Lpt and Za Simulations
In Quest of Devising Tools of Probing Cosmology and Gravity Using Galaxy Clusters
Dark Matters at the IFTUAM
Halo Concentrations in the Standard ΛCDM Cosmology
Halo and Subhalo Demographics with Planck Cosmological Parameters
Diapositiva 1
Cosmological Simulations of Galaxy Formation
Jhep04(2016)154
Supercdms Update
Cosmology and the Local Group in ΛCDM and Modified Gravity
PICASSO, COUPP and PICO
Arxiv:1109.0003V2 [Astro-Ph.CO] 2 Sep 2011
RHAPSODY: I. STRUCTURAL PROPERTIES and FORMATION HISTORY from a STATISTICAL SAMPLE of RE-SIMULATED CLUSTER-SIZE HALOS Hao-Yi Wu,1,2 Oliver Hahn,1 Risa H
Dark Matter Haloes and Subhaloes
Cold Dark Matter Plus Not-So-Clumpy Dark Relics
16Th Multidark Workshop -Program Abstracts
Milky Way's Satellites and the Cusp-Core Crisis
Multidark Was One of These 13 the Main Goal of Multidark Is to Contribute to the Identification and Detection of the Dark Matter
Data-Driven Modeling of Electron Recoil Nucleation in PICO C3F8 Bubble Chambers